Spectroscopic binaries near the north Galactic pole. XVII - HD 111425

Details Spectroscopic binaries near the north Galactic pole. XVII - HD 111425 Spectroscopic binaries near the north Galactic pole. XVII - HD 111425

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989japa...10..439g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 10, Dec. 1989, p. 439-443.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Northern Sky, Radial Velocity, Celestial Mechanics, Periodic Variations, Stellar Orbits

Scientific paper

Photoelectric radial-velocity measurements of HD 111425 from May 1980 to
March 1988 are presented. The observations show that the source is a
double-lined spectroscopic binary. It is found that the components of
the binary have types of about F8 V and G6 V and are in a 51-day orbit
of moderate eccentricity.

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